Second submission
1931607640
Assigned ID: 407
----- Attempting Submission 1 (Fri Apr 11 09:15:09 GMT 2014) -----
HST Phase I Proposal 407 (alma-followup.apt) successfully submitted.
----- Attempting Submission 2 (Fri Apr 11 17:58:09 GMT 2014) -----
0
----- Attempting Submission 1 (Fri Jul 25 00:35:06 GMT 2014) -----
A Detailed Dynamical And Morphological Study Of 5<z<6 Star, Dust, and Galaxy Formation With ALMA And HST
We propose WFC3-IR imaging for a unique sample of 10 ~L* "normal" 5<z<6 galaxies for which direct dust dust continuum emission and dynamical measurements from the CII 158um line obtained with ALMA. This is the first, and currently only sample of z~5-6 "normal" galaxies with direct and robust measurements of their dust content, star formation rates, and dynamics. These objects will provide a representative sample of galaxies in the primordial universe that will be used for a wide range of studies. Furthermore, the dense spectroscopic sampling at z>5 from Keck and VLT along with the wealth of multi-wavelength data in the proposed COSMOS field ensure the physical properties and local environment of these sources is known.
Immediate studies with the proposed WFC3-IR data include: 1) Measuring the rest-frame Ultraviolet (UV) spectral slopes to calibrate the infrared-excess - UV-slope (IRX-beta) relation which is an essential ingredient in estimating star formation rates at z>5 (e.g. Bouwens et al. 2012, Finkelstein et al. 2012), but is currently determined at z~0-2 and expected to strongly evolve at higher redshift (Meurer et al. 1999, Reddy et al. 2010,2012). 2) Compare quantitative morphologies with the ALMA dynamical measurements, constraining the formation mechanisms of these galaxies. 3) Significantly improve the spectra-energy distribution fits used to estimate stellar masses, which when combined with the dynamical mass estimates and atomic line data will test for biases in the mass estimates.
We are aiming to image 10 z~5-6 galaxies that have dust continuum and dynamical measurements from ALMA. The primary goal is to obtain WFC3-IR images in F105W, F125W and F160W to create resolved color maps of the galaxies in the rest frame UV. For Object 6 we are relying on existing observatios in F125W and F160W from program 13641 and changed the position of the F105W observations in this program by a few arc-seconds to match those.
We set up the observations to provide 4 dithered images so that Drizzel can better recover the galaxy morphology. A custom patter was used so that we could optimize the exposure time within each orbit.
The parallel obserations with ACS are designed to match similar data in the field obtaind by CANDELS and COSMOS. These consist of 1 orbit of F475W, 5/4 orbit of F606W, and 3/4 orbit of F814W to select dropout galaxies. In three cases (Visit 1, 3, and 6) it is possible to constrain the roll angle of the WFC3 observations such that the ACS FOV covers another object of interest. In these cases we took 1 orbit of F850LP which gives us an additional data point for our morphological constraint, an orbit of F814W to get a better Ly-alpha morphology, and the usual F606W which lets us select faint high-z objects at redshifts similar to our targets in the feilds.
UNRESOLVED STELLAR POPULATIONS AND GALAXY STRUCTURE
Default
false
false
false
false
false
SUPPORTED
GALAXY
HIGH REDSHIFT GALAXY
PROTOGALAXY
J2000
J2000
z=24.6, H=24.2
GALAXY
HIGH REDSHIFT GALAXY
PROTOGALAXY
J2000
J2000
z=24.8 H=24.2
GALAXY
HIGH REDSHIFT GALAXY
PROTOGALAXY
J2000
J2000
z=24.9 H=24.4
GALAXY
HIGH REDSHIFT GALAXY
PROTOGALAXY
J2000
J2000
z=24.5 H=23.8
GALAXY
HIGH REDSHIFT GALAXY
PROTOGALAXY
J2000
J2000
z=23.8 H=22.9
GALAXY
HIGH REDSHIFT GALAXY
PROTOGALAXY
Original Co-ordinates were 10:00:21.51, 2:35:10.90 changed to 10:00:20.3 , 2:35:20.5 to match previous deep observations from program 13384 in F125W and F160W and to obtain a second candiate in the field of view. Note this is not an exact match to the 13384 co-orinates of 10:00:20.7 , 2:35:20.5 due to the slightly different dither patern.
J2000
J2000
z=25.4 H=25.1
GALAXY
HIGH REDSHIFT GALAXY
PROTOGALAXY
J2000
J2000
z=24.6 H=24.1
GALAXY
HIGH REDSHIFT GALAXY
PROTOGALAXY
J2000
J2000
z=24.4 H=24.1
GALAXY
HIGH REDSHIFT GALAXY
PROTOGALAXY
J2000
J2000
z=24.9 H=24.3
GALAXY
HIGH REDSHIFT GALAXY
PROTOGALAXY
J2000
J2000
z=24.8 H>24.5
WFC3/IR
Imaging
No
No
F125W
WFC3/IR
Imaging
No
No
F160W
WFC3/IR
Imaging
No
No
F105W
WFC3/IR
Imaging
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No
F125W
WFC3/IR
Imaging
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No
F160W
WFC3/IR
Imaging
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F105W
WFC3/IR
Imaging
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No
F125W
WFC3/IR
Imaging
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No
F160W
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No
F105W
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F125W
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No
F160W
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No
F105W
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No
F105W
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No
F125W
WFC3/IR
Imaging
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No
F160W
WFC3/IR
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No
F105W
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No
F125W
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F160W
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No
F125W
WFC3/IR
Imaging
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No
F160W
WFC3/IR
Imaging
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No
F105W
WFC3/IR
Imaging
No
No
F125W
WFC3/IR
Imaging
No
No
F160W
WFC3/IR
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No
F105W
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Imaging
No
No
F125W
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Imaging
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No
F160W
WFC3/IR
Imaging
No
No
F105W
ACS/WFC
Imaging
No
No
F475W
ACS/WFC
Imaging
No
No
F606W
ACS/WFC
Imaging
No
No
F814W
ACS/WFC
Imaging
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No
F475W
ACS/WFC
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F606W
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F814W
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F475W
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F814W
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No
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No
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No
F475W
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No
F606W
ACS/WFC
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No
F814W
ACS/WFC
Imaging
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No
F475W
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No
F606W
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No
F814W
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No
F475W
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No
F606W
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No
F814W
ACS/WFC
Imaging
No
No
F475W
ACS/WFC
Imaging
No
No
F606W
ACS/WFC
Imaging
No
No
F814W
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:internal-dur-at-end 0
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 3222
:pcs-gap 0
)
(Tic-Orbit
:proposal-id 13641
:visit-id "09"
:orbit-number 3
:pcs-time 222
:si-vis-utilization 3000
:al-overhead-at-end 0
:internal-dur-at-end 980
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 3222
:pcs-gap 0
)
true
3
0
/Volumes/fastscr/Dropbox/Dropbox/OP-cache/hst-v10.xml
The scheduling data was generated by CASM 22.2.
CASM was run in Phase II mode.
(Tic-Visit
:proposal-id 13641
:visit-id "10"
:proposal-version -1
:trans-version "20140605"
:date "24-Jul-2014 17:23:05.0"
:trans-errors '(:WARNINGS 0 :ERRORS 0 :HEALTH-AND-SAFETY 0
:FATAL-ERRORS 0 :CONTINUABLE-FATALS 0)
:number-of-orbits 3
:saa-model "30"
:si-bright-earth-limb-angle 20.0
:data-volume 5221232
:tdrss-contact-duration 0
:coron NIL
)
(Tic-Obset
:proposal-id 13641
:visit-id "10"
:obset-id "10"
:pcs-mode "FGS"
)
(Tic-Orbit
:proposal-id 13641
:visit-id "10"
:orbit-number 1
:pcs-time 333
:si-vis-utilization 2889
:al-overhead-at-end 0
:internal-dur-at-end 0
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 3222
:pcs-gap 0
)
(Tic-Orbit
:proposal-id 13641
:visit-id "10"
:orbit-number 2
:pcs-time 222
:si-vis-utilization 3000
:al-overhead-at-end 0
:internal-dur-at-end 0
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 3222
:pcs-gap 0
)
(Tic-Orbit
:proposal-id 13641
:visit-id "10"
:orbit-number 3
:pcs-time 222
:si-vis-utilization 3000
:al-overhead-at-end 0
:internal-dur-at-end 980
:dark-offset NIL
:dark-utilization 0
:max-dark-utilization 1920
:low-sky "N"
:pcs-visibility 3222
:pcs-gap 0
)
true
3
0